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DTSTART;TZID=Europe/Rome:20191210T114500
DTEND;TZID=Europe/Rome:20191210T124500
DTSTAMP:20260507T133226
CREATED:20190723T112945Z
LAST-MODIFIED:20191204T155611Z
UID:6537-1575978300-1575981900@www.oa-roma.inaf.it
SUMMARY:Characterizing multi-phase gas outflows and their powering mechanism in nearby AGN
DESCRIPTION:Active Galactic Nuclei are thought to play a crucial role in\nthe evolution of massive galaxies. In particular\, fast outflows are\nfrequently observed in AGN covering various gas phases which may remove\na significant fraction of the gas content from the galaxies. I will\nreview the current state of research in this very active field of\nongoing research together with the advantages and disadvantages of\nprevious approaches. In particular\, I will highlight the importance of\nmulti-wavelength observations to unravel the true multi-phase nature of\noutflows by combining state-of-the-art observational facilities. In this\ncontext I will present the first results from the ongoing Close AGN\nReference Survey (CARS)\, a multi-wavelength survey of 39 luminous\nlow-redshift unobscured AGN with extensive observations from VLT/MUSE\,\nALMA\, VLA\, Chandra\, SOFIA and many more. In addition\, I will present the\nmulti-phase view of the famous ultra-luminous Quasar 3C273 where we\nunlocked a few unknown secrets.
URL:https://www.oa-roma.inaf.it/event/colloquium-bernd-husemann/
LOCATION:Aula Gratton
CATEGORIES:Seminari
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